5XMM J005744.6-722121

5XMM-DR15 stacked source · SRCID 3001854010101129
Position: 00h57m44.66s -72d21m21.7s (14.43609°, -72.35601°)
EP flux
1.23e-14 ± 1.8e-15 erg cm-2 s-1
CLASSX
AGN (0.855)
Detections
21

SRCID 3001854010101129
IAUNAME 5XMM J005744.6-722121
SC_RA 00h57m44.66s (14.43609°)
SC_DEC -72d21m21.7s (-72.35601°)
RADEC_ERR 0.59 arcsec
LII / BII 302.2589° / -44.7640°
N_CONTRIB 21 (detections)
N_OBS 182 (observations covering the position)
MJD_FIRST 51834.632 (2000-10-17 15:10:35.000 UTC)
MJD_LAST 58925.579 (2020-03-17 13:54:08.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.23e-14 ± 1.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.77 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.52 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.19 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.41 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.974

Class probabilities
Class taxonomy
  • AGN — active galactic nucleus.
  • Bkg_AGN — background AGN.
  • Star — Galactic star.
  • Gal_XRB — Galactic X-ray binary.
  • Extragal_XRB — extragalactic X-ray binary.
  • CV — cataclysmic variable.
  • Extended — cluster or galaxy.

Optical Monitor (OM)
OM Source ID
366032
Match probability
0.631
FilterMag (AB)Err
UVW2 18.162 0.064
UVM2 18.078 0.035
UVW1 17.978 0.014
U
B 17.648 0.014
V
Gaia DR3
Source ID
4689000308934375680
Match probability
0.985
Parallax
-0.104 ± 0.123 mas
Proper motion
(0.13, -1.44) mas/yr
Magnitudes
G=18.29, BP=18.19, RP=18.31
Distance
21448 pc
CLASSOPT
Class
QSO
Star
0.00
AGN
0.94
Galaxy
0.06

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 7.42e-15 (+1.1e-14 / −4.8e-15) erg cm−2 s−1
NH 2.74e+21 (+1.8e+22 / −1.2e+20) cm−2
Photon index (Γ) 1.44 (+2.24 / −1.11)
DoF 151
p-value 0.643
Quality flag 0

APPROX_SOURCE_VAR 6.200 (approximate flux variability amplitude)

No contributing observations found.

Sky view (optical)

DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.

Hardness-ratio diagram

The per-observation light curve is shown in the X-ray properties section above.